2000/11/17 by Jaan Einasto, Einasto, Jaan
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0011334
LaTex (sty files added), 10 pages, 5 PostScript figures embedded, in ``9th Marcel Grossmann Meeting on relativistic astrophysics'', ed. R. Ruffini, World Scientific, Singapore (in press)
arxiv created 2000/11/17 · arxiv updated 2009/12/01
Observational evidence for the presence of a preferred scale around 100 Mpc in the distribution of high-density regions in the Universe is summarised. Toy models with various degrees of regularity are analysed to understand better the observational data. Predictions of models which produce a feature on the initial power spectrum of matter are analysed and compared with new observational data on the CMB angular spectrum, cluster mass function, and galaxy and cluster power spectrum.